| Observation data Epoch J2000 Equinox ICRS | |
|---|---|
| Constellation | Mensa |
| Right ascension | 04h 54m 48.292s |
| Declination | −76° 40′ 49.89″ |
| Characteristics | |
| Evolutionary stage | subgiant |
| Spectral type | G9IV |
| Astrometry | |
| Proper motion (μ) | RA: 11.849±0.013 mas/yr Dec.: −18.732±0.013 mas/yr |
| Parallax (π) | 2.8128±0.0105 mas |
| Distance | 1,160 ± 4 ly (356 ± 1 pc) |
| Details | |
| Mass | 0.923 M☉ |
| Radius | 1.0977 R☉ |
| Luminosity | 1.106 L☉ |
| Surface gravity (log g) | 4.3027 cgs |
| Temperature | 5629 K |
| Age | 12.82+0.73 −1.40 Gyr |
| Other designations | |
| 2MASS J04544830-7640498, TIC 140691463, Gaia DR3 4624979393181971328 | |
| Database references | |
| SIMBAD | data |
TOI-157 (also known as TIC 140691463) is a G-type subgiant star located about 1160 light years (356 pc) from Earth. It has a mass of about 0.92 solar masses, a radius of about 1.1 solar radii and a temperature of about 5600 K. It is approximately 12.0 to 12.8 billion years old.
It has one discovered exoplanet orbiting it named TOI-157b. It is a gas giant classed as a hot Jupiter with a mass of 1.18 Jupiter masses and a radius of 1.286 Jupiter radii. It orbits very close to the star taking only 2 days to complete an orbit. This places the temperature of TOI-157b to be around 1588 Kelvin. Using TESS data discrepant transit parameters as well as empirical limb-darkening coefficients could be determined. Further analysis revealed that the radius ratio of planet to star is 7.8 ± 0.4 % higher than previously determined, caused by blending with the light from background stars, at a new value of 0.1229 ± 0.0005.
It is a typical hot Jupiter. However, at an age of 12.82+0.73
−1.4 billion years the planet is currently the oldest discovered and only about 1 billion years younger than the age of the universe at about 13.8 billion years. Only PSR B1620-26 b with 11.2–12.7 Gyr remains as alternatively oldest exoplanet.